-unbound levels in from reaction measurements and implications for the astrophysical reaction rate
Abstract
The reaction has been identified in several type-1 x-ray burst (XRB) sensitivity studies as a significant reaction within the
- Authors:
-
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- Univ. of Notre Dame, IN (United States); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Tohoku Univ., Sendai (Japan)
- Univ. of Notre Dame, IN (United States)
- Kyushu Univ. (Japan)
- Osaka Univ. (Japan)
- Niigata Univ. (Japan)
- Univ. of Notre Dame, IN (United States); Argonne National Lab. (ANL), Lemont, IL (United States)
- Florida State Univ., Tallahassee, FL (United States)
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1524392
- Alternate Identifier(s):
- OSTI ID: 1438271
- Report Number(s):
- LA-UR-17-31506
Journal ID: ISSN 2469-9985; PRVCAN
- Grant/Contract Number:
- 89233218CNA000001; PHY-1068192; SC0009883
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 97; Journal Issue: 5; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Atomic and Nuclear Physics; Astronomy and Astrophysics
Citation Formats
Long, Alexander Makenzie, Adachi, T., Beard, M., Berg, G. P. A., Couder, M., deBoer, R. J., Dozono, M., Görres, J., Fujita, H., Fujita, Y., Hatanaka, K., Ishikawa, D., Kubo, T., Matsubara, H., Namiki, Y., O'Brien, S., Ohkuma, Y., Okamura, H., Ong, H. J., Patel, D., Sakemi, Y., Shimbara, Y., Suzuki, S., Talwar, R., Tamii, A., Volya, A., Wakasa, T., Watanabe, R., Wiescher, M., Yamada, R., and Zenihiro, J. α -unbound levels in Ar34 from Ar36(p,t)Ar34 reaction measurements and implications for the astrophysical S30(α,p)Cl33 reaction rate. United States: N. p., 2018.
Web. doi:10.1103/PhysRevC.97.054613.
Long, Alexander Makenzie, Adachi, T., Beard, M., Berg, G. P. A., Couder, M., deBoer, R. J., Dozono, M., Görres, J., Fujita, H., Fujita, Y., Hatanaka, K., Ishikawa, D., Kubo, T., Matsubara, H., Namiki, Y., O'Brien, S., Ohkuma, Y., Okamura, H., Ong, H. J., Patel, D., Sakemi, Y., Shimbara, Y., Suzuki, S., Talwar, R., Tamii, A., Volya, A., Wakasa, T., Watanabe, R., Wiescher, M., Yamada, R., & Zenihiro, J. α -unbound levels in Ar34 from Ar36(p,t)Ar34 reaction measurements and implications for the astrophysical S30(α,p)Cl33 reaction rate. United States. https://doi.org/10.1103/PhysRevC.97.054613
Long, Alexander Makenzie, Adachi, T., Beard, M., Berg, G. P. A., Couder, M., deBoer, R. J., Dozono, M., Görres, J., Fujita, H., Fujita, Y., Hatanaka, K., Ishikawa, D., Kubo, T., Matsubara, H., Namiki, Y., O'Brien, S., Ohkuma, Y., Okamura, H., Ong, H. J., Patel, D., Sakemi, Y., Shimbara, Y., Suzuki, S., Talwar, R., Tamii, A., Volya, A., Wakasa, T., Watanabe, R., Wiescher, M., Yamada, R., and Zenihiro, J. Tue .
"α -unbound levels in Ar34 from Ar36(p,t)Ar34 reaction measurements and implications for the astrophysical S30(α,p)Cl33 reaction rate". United States. https://doi.org/10.1103/PhysRevC.97.054613. https://www.osti.gov/servlets/purl/1524392.
@article{osti_1524392,
title = {α -unbound levels in Ar34 from Ar36(p,t)Ar34 reaction measurements and implications for the astrophysical S30(α,p)Cl33 reaction rate},
author = {Long, Alexander Makenzie and Adachi, T. and Beard, M. and Berg, G. P. A. and Couder, M. and deBoer, R. J. and Dozono, M. and Görres, J. and Fujita, H. and Fujita, Y. and Hatanaka, K. and Ishikawa, D. and Kubo, T. and Matsubara, H. and Namiki, Y. and O'Brien, S. and Ohkuma, Y. and Okamura, H. and Ong, H. J. and Patel, D. and Sakemi, Y. and Shimbara, Y. and Suzuki, S. and Talwar, R. and Tamii, A. and Volya, A. and Wakasa, T. and Watanabe, R. and Wiescher, M. and Yamada, R. and Zenihiro, J.},
abstractNote = {The S30(α,p)Cl33 reaction has been identified in several type-1 x-ray burst (XRB) sensitivity studies as a significant reaction within the α,p process, potentially influencing not only the abundances of burst ashes but also the bolometric shape of double-peaked light curves coming from certain XRB systems. Given the dearth of experimental data on the S30(α,p)Cl33 reaction at burst temperatures, we have performed high energy-resolution forward-angle Ar36(p,t)Ar34 measurements in order to identify levels in 34Ar that could appear as resonances in the S30(α,p)Cl33 reaction Energies of levels identified in this research, along with model-based assumptions for spin assignments and spectroscopic factors, were then used to determine a rate for the S30(α,p)Cl33 reaction based on a narrow-resonance formalism. The rates determined in this work are then compared with two standard Hauser-Feshbach model predictions over a range of XRB temperatures.},
doi = {10.1103/PhysRevC.97.054613},
journal = {Physical Review C},
number = 5,
volume = 97,
place = {United States},
year = {Tue May 22 00:00:00 EDT 2018},
month = {Tue May 22 00:00:00 EDT 2018}
}
Web of Science
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